The physical properties of the system were calculated using the \(r_{\rm A}\) , \(r_{\rm B}\)  and \(i\)  from Table REF , the orbital period determined above, and the final \(K_{\rm A}\)  and \(K_{\rm B}\)  values from Table REF . We used standard formulae [1]} and the reference solar values from the IAU [2]}, as implemented in the jktabsdim code [3]}. The results are given in Table REF  and show good news: the masses are measured to precisions of 0.8% and 0.5%, and the radii to 0.5% and 0.4%. The main limitation is the lower precision of \(K_{\rm B}\) , which is in turn due to the minor disagreement between the two sources of published RVs.
